FREE BOOKS

Author's List




PREV.   NEXT  
|<   242   243   244   245   246   247   248   249   250   251   252   253   254   255   256   257   258   259   260   261   262   263   264   265   266  
267   268   269   270   271   272   273   274   275   276   277   278   279   280   281   282   283   284   285   286   287   288   289   290   291   >>   >|  
effect lasted in some instances as long as an hour and three-quarters after sunset. In India the sun and skies assumed a greenish hue, and there was much curiosity regarding the cause of the "green sun." Another remarkable phenomenon of this period was the great prevalence of rain during the succeeding winter. This probably was due to the same cause; that is, to the fact of the air being so filled with dust; the prevailing theory in regard to rain being that the existence of dust in the air is necessary to its fall. The vapor of the air concentrates into drops around such minute particles, the result being that where dust is absent rain cannot fall. As regards the sunsets spoken of, there are three similar instances on record. The first of these was in the year 526, when a dry fog covered the Roman Empire with a red haze. Nothing further is known concerning it. The other instances were in the years 1783 and 1831. The former of these has been traced to the great eruption of Skaptur Jokull in that year. It lasted for several months as a pale blue haze, and occasioned so much obscurity that the sun was only visible when twelve degrees above the horizon, and then it had a blood-red appearance. Violent thunderstorms were associated with it, thus assimilating it with that of 1883. Alike in 1783 and 1831 there was a pearly, phosphorescent gleam in the atmosphere, by which small print could be read at midnight. We know nothing regarding the meteorological conditions of 1831. The red sunsets of 1883 were remarkable for their long persistence. They were observed in the autumn of 1884 with almost their original brilliancy, and they were still visible in 1885, being seen at intervals, as if the dust was then distributed in patches, and driven about by the winds. In fact, similar sunsets were occasionally visible for several years afterwards. These may well have been due to the same cause, when we consider with what extreme slowness very fine dust makes its way through the air, and how much it may be affected by the winds. THE RED SUNSETS DESCRIBED One writer describes the appearance of these sunsets in the following terms: "Immediately after sunset a patch of white light appeared ten or fifteen degrees above the horizon, and shone for ten minutes with a pearly lustre. Beneath it a layer of bright red rested on the horizon, melting upward into orange, and this passed into yellow light, which spread around the lucid spot.
PREV.   NEXT  
|<   242   243   244   245   246   247   248   249   250   251   252   253   254   255   256   257   258   259   260   261   262   263   264   265   266  
267   268   269   270   271   272   273   274   275   276   277   278   279   280   281   282   283   284   285   286   287   288   289   290   291   >>   >|  



Top keywords:

sunsets

 

instances

 

horizon

 
visible
 

degrees

 
similar
 

lasted

 

sunset

 

appearance

 
pearly

remarkable

 

midnight

 

driven

 

distributed

 

patches

 

original

 

autumn

 
observed
 
persistence
 
conditions

brilliancy

 

intervals

 
meteorological
 

affected

 

fifteen

 

minutes

 

lustre

 
appeared
 

Immediately

 

Beneath


yellow

 

spread

 

passed

 

orange

 

bright

 

rested

 

melting

 
upward
 

describes

 
extreme

slowness

 

SUNSETS

 

DESCRIBED

 

writer

 

occasionally

 

Skaptur

 

existence

 

concentrates

 

regard

 

theory